Talk:HD 112028
 | This article is rated Start-class on Wikipedia's content assessment scale. It is of interest to the following WikiProjects: | |||||||||||||
| ||||||||||||||
.jpg){kind=small}
Confusal with https://en.wikipedia.org/wiki/Struve_1694?
editThis page is identical in some ways with https://en.wikipedia.org/wiki/Struve_1694
Both Σ 1694 A and HD 112028 are catalogued under HR 4893. Σ 1694 B, however, is catalogued under HR 4892 and HD 112014. Confusingly, https://en.wikipedia.org/wiki/HD_112028 does not cite Struve 1694 as an alternate designation.
On https://en.wikipedia.org/wiki/HD_112028, both components are stated to be at a distance of approx. 600 LY. On https://en.wikipedia.org/wiki/Struve_1694, Σ 1694 A is stated to be at a distance of approx. 310 LY, whilst Σ 1694 B stated to be at a distance of approx. 200 LY.
Astronomical statistics otherwise match on both pages regarding Σ 1694 A, and the spectral types match for both Σ 1694 A and Σ 1694 B.
Are we looking at the same star here? If so, I propose that the articles be merged and conflicting data be investigated. — Preceding unsigned comment added by 88.109.188.99 (talk) 14:15, 15 July 2016 (UTC)
- Same star(s). Pick the better article, add any additional information to it that the other article might have. Then turn the redundant article into a redirect. Lithopsian (talk) 15:53, 19 July 2016 (UTC)